Dust ring and gap formation by gas flow induced by low-mass planets embedded in protoplanetary disks - I. Steady-state model

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Fig. E.2

Same as in Fig. E.1, but with m = 0.03 and M_hw = 0.1. The planet-induced gas flow is in the flow-headwind regime. The sphere is the Bondi sphere of the planet, whose size is 0.03 [H]. The vertical dashed line in panel c corresponds to the x coordinate of the position of the corotation radius for the gas, x_g,cor = −2/3 M_hw.

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